Physics
Scientist
Crimean Astrophysical Observatory
Krymskaia Astrofizicheskaia Observatoriia, Nauchny, Ukrainian SSR
Krymskaya Astrofizicheskaya Observatoriya
Changes with Height of Longitudinal Magnetic Field in Active Regions
Comparison of observed and calculated magnetic field structures for a potential model for two active regions
Digital vector magnetograph. I. Longitudinal field channel.
Dynamics phenomena in active regions on the Sun
Height changes of parameters in the model of plasma flow in sunspot umbra above the temperature minimum region
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